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The Filament Eruption in the 3B Flare of July 29, 1973: Onset and Magnetic Field Configuration

Published online by Cambridge University Press:  14 August 2015

R. L. Moore  and
B.J. Labonte
R. L. Moore
Affiliation:
Caltech, Big Bear Solar Observatory, Hale Observatories
B.J. Labonte
Affiliation:
Hale Observatories

Extract

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We present direct observational evidence for the preflare magnetic field configuration, the nature of the filament destabilization and triggering of the flare, and the magnetic field configuration after the filament eruption in the large, well-ordered, expanding two-ribbon flare of July 29, 1973.

Type
Part III. Solar Transient Phenomena Affecting the Corona and Interplanetary Medium: Dynamics Deduced from Observations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 207 - 211
Copyright
Copyright © Reidel 1980 

References

Heyvaerts, J., Priest, E.R., and Rust, D.M.: 1977, Astrophys J 216, pp. 123–137.Google Scholar
Hirayama, T.: 1974, Solar Phys 34, pp. 323–338.CrossRefGoogle Scholar